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Table 4

Estimates for λ0 and f0 of Hα both from our TPV method and independent methods.

ID a zCOSMOS b pairc λ0d (TPV) λ0d (spec) λ0d,f (phot-z) fHαe (TPV) fHαe ([ O ii ]) fHαe (Hβ) fHαe (total) fHαe (SED)
7 810 332 15/16 1201.3 1201 16.5 ± 2.6 34.2 ± 5.2
14 15/16 1180
33 810 529 15/16 1199.1 1194 13.2 ± 2.3
94 14/15 1199
96 822610 14/15 1197.6 1186 11.3 ± 1.8
97 14/15 1204
99 822 560 14/15 1189.9 1191 2.4 ± 0.9
104 14/15 1201
105g,h 822 732 14/15 1199.4 AGN 2.4 ± 0.4 24.7 ± 8.6
111 14/15 1197
113 823 319 14/15 1197.7 1186 5.0 ± 1.1 7.1 ± 2.6
114 822686 14/15 1193.2 1190 9.6 ± 1.7
117g 822 508 14/15 1194.7 AGN 11.2 ± 2.5
121 822 822 14/15 1197.3 1174 23.3 ± 3.9 33.5 ± 6.5
122 14/15 1197
124 14/15 1188
125 822 496 14/15 1198.5 1190 4.6 ± 1.1
126 14/15 1199
128 14/15 1162
131 14/15 1201
135i 823 097 14/15 1184.5 11.8 ± 1.9 25.3 ± 7.5
138 822 504 14/15 1195.0 1186 19.4 ± 2.9 20.4 ± 4.6
147 14/15 1153
150 14/15 1188
153 14/15 1182
161 14/15 1211
164 14/15 1184
167 823 087 14/15 1191.7 30.4 ± 3.4 46.3 ± 8.5
170 14/15 1186
172 09/10 1180
186 839 235 09/10 1197.6 1104 9.1 ± 2.7 17.8 ± 6.2
204 838 539 09/10 1182.3 1141 4.4 ± 2.2
205 838 552 09/10 1181.6 1180 6.9 ± 1.4
226 09/10 1201
235 09/10 1185

Notes. The independent estimates are based on conversions from zCOSMOS [O ii] and Hβ fluxes (cf. Sect. 5.6.3), on Hα estimates from SED fitting (cf. Sect. 5.6.1), and on SFR estimates from the combination of UV + IR (cf. Sect. 5.6.2). As an example, cutouts for objects 121 and 135 are shown in Fig. 12. Properties of the best-fit SEDs and the EWobs from the TPV are given in Appendix E as part of the supplementing Table E.1.

(a)

NBES;

(b)

zCOSMOS bright 20k (Lilly et al. 2009) ID;

(c)

Contributing NB118 filters.

(d)

Hα central wavelength [nm];

(e)

[10-17 ergs-1cm-2];

(f)

Redshifts from Ilbert et al. (2013).

(g)

Chandra point source (Civano et al. 2012);

(h)

zCOSMOS confidence class 13.5 (BL AGN);

(i)

[Ne v]λ3426 detected in zCOSMOS spectrum.

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